54348510 Modern Physics

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    Modern Physics

    An excursion into the

    development of new ideas

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    BBRThings to know

    What is a black body

    Sketch the spectrum of BB at different

    temperatures

    Note that

    Wavelength at peak intensity (lmax)

    decreases with increase temperature

    Relationship lmaxis proportion to absolute

    Temperature Wiens law (constant 2.898x10-3 m.K)

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    Black Body Radiation

    http://rh5.clemson.edu/ropermtn/naturalEM.php

    Credits

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    Total power per unit area is the area under the curve

    This increases with temperature

    Stefans law gives the relationship (P = eAs T4) I = sT4

    Rayleigh-Jean Law

    Attempt to derive spectral intensity by considering

    standing waves in the cavity

    Ultraviolet catastrophe (small wavelength)

    Infinite total power

    4

    2),(

    l

    l

    TkcTI B

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    Plancks Solution

    Assumptions Cavity Walls are oscillators

    Oscillators have range of fundamental

    frequencies Oscillators exchange radiation with cavity

    Each oscillator of fund. Freq. f can absorb or

    emit energy

    E = n h f where n = 0,1,2,3

    Novel Idea

    Led to the correct eqn

    1

    2),(

    5

    2

    Tk

    hc

    Be

    hcTI

    ll

    l

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    Photoelectric Effect

    http://www.physics.umd.edu/perg/qm/qmcourse/NewModel/research

    /pe_jcmst/Jcmst00.htm

    Credits

    http://www.physics.umd.edu/perg/qm/qmcourse/NewModel/researchhttp://www.physics.umd.edu/perg/qm/qmcourse/NewModel/research
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    Classical Expectations

    Light is a wave so its energy must dependon the intensity and independent of itsfrequency.

    Emission of photoelectrons should notdepend on the frequency, but on theintensity

    KE should depend on its intensity A delay should be expected as electrons

    absorb enough energy from the wave

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    Graphs

    http://library.thinkquest.org/28383/nowe_teksty/htmla/1_8a.html

    Credits

    http://phycomp.technion.ac.il/~webteach/phys3/ph114053/adler/photo.html

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    Observations

    No current for frequency below threshold (Cutoff)

    frequency. Independent of intensity

    The amount of saturation current depends on the light

    intensity

    The maximum kinetic energy (or stopping voltage ) is

    proportional to frequency, independent of intensity

    Threshold frequency depends on the metal

    Stopping voltage depends only on metal and frequency ,not on intensity

    Instantaneous emission of electrons on illumination

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    Conclusions

    Light consists of discrete photons

    Energy of a photon E = hf

    Atom absorbs total photon Energy equal to the work function needed

    to remove electron from atom

    WF depends on the metal used Energy of photon in excess of WF goes

    into K.E of electron (Cons. Of Energy)

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    Compton Effect

    Monochromatic X-rays scattered fromelectrons in Graphite

    Observed change in wavelength which

    varied with scattering angle (not expected)

    )cos(112 ll cm

    h

    e

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    Diagram

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    Explanation

    Light consists of discrete particles

    These particles collide with the stationary

    electrons of the graphite

    Relativistic energy and momentum are

    conserved (similar to particle-particle

    collision)

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    The Sun emits energy at a rate of 3.9x1026

    W.(i) If the radius is 6.96x108 m, determinethe mean temperature.(ii) If the average

    wavelength of its radiation is 550 nm,

    determine the average number of photons

    emitted by the sun in a second.

    The wavelength associated with the cutoff

    frequency of silver is 325 nm. Find themaximum kinetic energy and the stopping

    potential for electrons emitted when silver is

    illuminated by ultraviolet light of wavelength

    Class Exercises

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    Atomic Spectra Sunlight has continuous spectrum

    When electric arc passed through gas, the gas

    emits a line (emission) spectrum

    White light passing through low density gas resultsin absorption spectrum

    http://academic.kellogg.cc.mi.us/herbrandsonc/bio111/metabolism.htm

    www.prophotolife.com

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    Atomic Spectra

    http://www.ruf.rice.edu/~mcannon/Research%20Home/Research%20Home%20Pictures/Spectrum.jpg

    The Absorption and

    emission spectraare characteristic of the

    element.

    Applications:Study of elements in The

    Sun and Stars

    Analysis of heavy metal

    contamination in food

    Neon Signs

    Fluorescent lamps

    http://www.ruf.rice.edu/~mcannon/Research%20Home/Research%20Home%20Pictures/http://www.ruf.rice.edu/~mcannon/Research%20Home/Research%20Home%20Pictures/
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    Spectral Series of Hydrogen

    RH is Rhdberg constant = 1.097373x107 m-1

    nf = 2 Balmer series ( first observed and equation

    deduced by school teacher)

    nf = 1 Lyman series (UV range)

    nf = 3 Paschen Series

    Note ni > nf

    Note n 0

    Equation was empirical (not based on Theory)

    22

    111

    if

    Hnn

    Rl

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    Bohrs Postulates

    Atom consists of electrons in circular orbits around

    positive nucleus with Newtonian physics applying to

    orbit.

    The electron can only exist in stationary states. In these

    states no energy is emitted

    If an electron moves from one stationary state to that of

    lower energy a photon is emitted with

    E1 - E2 = h f (f is the frequency of the photon) The stationary states are such that angular momentum is

    quantised mvr = n h/2(pi) n = 1,2,3,4,.

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    Derivation of Bohrs atom

    Coulomb Force Centripetal Acceleration

    Energy E = PE + KE

    Fourth Postulate

    Obtain

    rn = a n2

    a = 52.92 pm En= 13.60 eV /n2

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    Class Exercises

    Determine the energy required to ionise a

    hydrogen atom from the state n= 3. A

    photon transitions from n=6 to n= 2.

    Calculate the (i) Energy (ii) Wavelength ofthe emitted photon.

    Discuss ground state, excited states

    Draw the energy level diagram, theionisation energy and the first Bohr radius

    for Singly ionised helium (-54.4eV n =1)

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    Limitations of Bohr Atom

    The Bohr Model

    has flat circle but observation shows spherical

    electronic orbit

    Has minimum angular momentum of h/2

    however Lmin = 0 Cannot explain spectra of more complex atoms

    Cannot account for the variation of intensity or

    splitting of spectral line under magnetic fields Cannot account for the wave nature of the

    electron

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    Nature of Light

    Interference of light seemed conclusiveevidence for wave nature of light

    Photoelectric effect discrete localised

    energy Compton Effect proved localised p, E

    Both confirm particle nature of light

    Reduce light intensity in Youngsexperiment

    Individual particles detected on screen

    Conclude wave-particle duality for light

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    De Broglie

    Particle has a wavelength = h/p

    Observed by Davisson Germer

    Interference pattern observed for e, p, n, I2& buckyballs

    Applications

    Electron & Neutron diffraction used todetermine atomic structure liquids &solid

    Electron diffraction used to study surfaces of

    solids

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    Class Exercises

    In the typical television set the electrons

    are accelerated through a potentialdifference of 25.0kV. Ignoring relativistic

    effect, determine their De Broglie

    wavelength and compare it to that of atennis ball served by Serena Williams

    (m=56.7 g v= 120 mph)

    1 mph = 0.447 m/s

    p: www you u e com wa c v= e

    http://www.youtube.com/watch?v=ZUI3lhRje_0http://www.youtube.com/watch?v=ZUI3lhRje_0
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    p: www.you u e.com wa c v= e_

    Observe Individual particles at detector

    Low intensity area has low probabilityof particle

    Interference pattern emerge over

    time

    Deduce e- detected as particles, but their

    probability of arrival at a point on thescreen is determined by theinterference of a pair of waves

    Image Credit

    http://scienceblogs.com/startswithabang/upload/2009/05/

    a_tale_of_two_slits/electron_two_slit.jpg

    http://www.youtube.com/watch?v=ZUI3lhRje_0http://scienceblogs.com/startswithabang/upload/2009/05/http://scienceblogs.com/startswithabang/upload/2009/05/http://www.youtube.com/watch?v=ZUI3lhRje_0
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    Complimentarity

    The double slit experiment with reduced

    particle number showed that the electron

    is detected as a particle but their arrival at

    a point on the screen is determined by theinterference of two waves.

    Thus both wave and particle properties are

    required to explain the particle.

    Cannot observe both properties

    simultanteously

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    Cover one slit

    No interference

    http://www.youtube.com/watch?v=DfPeprQ7oGc

    http://www.youtube.com/watch?v=DfPeprQ7oGchttp://www.youtube.com/watch?v=DfPeprQ7oGchttp://www.youtube.com/watch?v=DfPeprQ7oGc
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    Quantum Mechanics

    Matter wave?

    Is complex

    Has everything knowable about particle

    Satisfy Schrdinger Equation

    Interpretation of wave function

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    Poetry in Physics Origin German

    Erwin kann mit seinem Psi

    kalkulieren wie noch nie.

    Doch wird jeder gleich einsehn:

    Psi lsst sich nicht recht verstehn

    English translation that does not run as

    smoothly, but may be easier to understand for

    some. :-)

    Erwin with his psi can docalculations quite a few.

    But one thing has not been seen:

    Just what does psi really mean?

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    What Psi means

    dxxdxxP2

    )()(

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    Review Standing Wave

    Standing wave on a string of length L

    l = 2L/n with n = 1,2,3

    Note wavelengths are quantised For standing wave y = sin(kx)

    Express y in terms of L & n

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    Particle in a box

    Particle in 1-D box with Infinitely hard walls Infinite potential well

    Width of well L

    Mass of particle m Particle exists only in certain stationary states

    Stationary states are standing waves

    Determines the possible wavelengths

    L = ln/2 n = 1,2,3

    The wave function is standing wave

    Wave-function defines the probability distribution

    of the particle

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    Quantised Energy Levels

    By DeBroglie the wavelength determines

    the momentum

    p determines KE for that state

    Recall V= 0 so total E =

    Derive E

    Only quantised energy possible Note n 0 thus lowest energy state n = 1

    ground state energy.

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    Wave Function for PiB

    Sketch

    (x)

    ||2

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    Class Exercises An electron is trapped in an infinite potential well

    (particle in 1-D box) 250 pm wide and is in the

    ground state. How much energy must it absorb if it is

    to jump to the state n = 4. Determine the wavelength

    of the photon emitted when it subsequently drops

    back down to the n = 2 energy level.

    A particle of mass m is in an infinite potential well of

    width L. The particle is in the first excited state. Findthe ratio of the probability of finding the particle in a

    small interval about point x = L/3 to that of finding

    the particle in an interval of equal size around the

    point x = L/4.

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    Black Body Radiation

    Temperature Wiens law

    Stefans law

    Plancks Solution

    Photoelectric Effect

    Experiment

    Classical Expectations

    Graphs

    Observations

    Einsteins Solution

    Compton Effect

    Experiment

    Results

    Explanation

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    Atomic Spectra

    Emission/Absorption

    Spectral Series of Hydrogen Bohrs Postulates

    Bohrs atom

    De Broglies Hypothesis Quantum Mechanics

    Wave function

    Wave function interpretation Particle in a box